From the marine refraction data recorded on five instruments during th
e Clipperton Area Seismic Survey to investigate Compensation (CLASSIC)
experiment in 1994 we construct a compressional velocity model for a
108 km long profile across the Clipperton transform. We apply a new se
ismic tomography code that alternates between ray tracing and lineariz
ed inversions to find a smooth seismic velocity model that fits the ob
served refraction travel times. The solution to the forward ray-tracin
g problem is a hybrid of the graph (or shortest path) method and a ray
-bending method. The inversion is performed with least squares penalti
es on the data misfit and first derivatives of the seismic structure.
Starting with a one-dimensional compressional velocity model for ocean
ic crust, the misfit in the normalized travel time residuals is reduce
d by 96%, decreasing the median travel time residual from 110 to 25 ms
. The compressional velocity structure of the Clipperton transform is
characterized by anomalously low velocities, about 1.0 km/s lower than
average, beneath the median ridge and parallel troughs of the transfo
rm domain. The low compressional velocities can be explained by an inc
reased porosity due to fracturing of the oceanic crust. We found crust
al thicknesses of 5.6-5.9 km under the transform fault to produce the
best fit of the PmP phase arrivals and Pg/Pn crossovers. Since the cru
st is not thin beneath the transform parallel troughs and the velocity
anomaly is not confined to the median ridge, we find uplift by serpen
tinite diapirs unlikely as an explanation for the relief of the median
ridge. A median ridge that is the result of brittle deformation due t
o compression across the transform domain is, however, compatible with
our results. The upper crust is thicker to the north of the transform
than to the south, which is likely a consequence of the contrast in t
emperature structure of these two spreading segments.